← atlas

6dFGS gJ183450.8-572422

Observation

Spectrum ID477842826_sp2
Alt nameg1834508-572422
z0.0548
RA, Dec278.7117, -57.4061
MJD60165.46
SNR/Å B/R12.9/20.3
Obs Airmass1.12
SMSS ID477842826
Closest SMSS11.62'', 1580175660
SMSS Mean r6"ap16.7 ± 0.1
2MASS Kext12.4 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.083
Power law αν-1.27 ± 0.25
log L5100,AGN42.29 ± 0.10
log HβBr/[O III]0.03 ± 0.06
log ML5100/M6.74 ± 0.14
log M/M6.38 ± 0.06
log M/M6.76 ± 0.14
log M[O III]/M6.86 ± 0.14

Spatial extraction & sky subtraction region

Spatial plot

Spaxel scale: 1 arcsec² — Flux units: erg s⁻¹ cm⁻² Å⁻¹
Apertures: object (solid), background (dashed)

Spectrum decomposition

Emission line measurements

Linelog L (erg s⁻¹)FWHM (km s⁻¹)σ (km s⁻¹)EW (Å)
Hγ Narrow39.37 ± 0.23226 ± 63280 ± 365.53 ± 3.41
Hγ Broad40.08 ± 0.132294 ± 229550 ± 2626.63 ± 5.11
[O III] 436439.00 ± 0.37213 ± 6390 ± 252.31 ± 1.40
He II Narrow
He II Broad39.63 ± 0.281984 ± 67842 ± 2710.45 ± 4.19
Hβ Narrow39.59 ± 0.16226 ± 63280 ± 369.79 ± 3.02
Hβ Broad40.58 ± 0.051919 ± 2771189 ± 8896.02 ± 6.47
[O III] 500740.55 ± 0.03226 ± 63280 ± 3691.21 ± 3.57
He I Narrow
He I Broad39.80 ± 0.141629 ± 72692 ± 2918.22 ± 3.36
[O I] 630039.04 ± 0.23213 ± 6390 ± 253.35 ± 1.17
Hα Narrow39.98 ± 0.05213 ± 6390 ± 2529.92 ± 1.48
Hα Broad41.07 ± 0.011659 ± 82803 ± 34368.93 ± 5.76
[N II] 658540.07 ± 0.03213 ± 6390 ± 2536.73 ± 1.48
[S II] 671839.60 ± 0.07213 ± 6390 ± 2512.63 ± 1.30
[S II] 673239.50 ± 0.09213 ± 6390 ± 2510.17 ± 1.28

All narrow line widths are tied to narrow [O III] 5007Å. [O III] 5007Å and narrow Hβ include a second narrow component not tied to other narrow lines.

Emission summary

Hα Broad SNR8.01
Hβ Broad SNR2.68
Hγ Broad SNR1.08
AGN frac0.10
Host frac0.90
log L5100,Host43.24
Fe II/Hβ0.45
Fe II/[O III]0.48

Quality flags

spurious_hab/hbb0.0/0
l51002
balmer1
balmer_snr1
hb_width1
balmer_width0

Hα mass estimates from Cho+2023. Remaining mass estimates from R–L relations in Wang & Woo 2024 and zero-points from Amrutha+2026.